CWNU 3592

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C3
N_50
r_50
AA 22 2.1
Summary

CWNU 3592 is a sparse, very loose object of very high C3 quality. It is located at a very large distance from the Sun, well below the mid-plane. It was recently reported in the literature.

Warning: contains less than 25 stars with P>0.5 estimated.

Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 242.565 -54.978 0.005 -2.871 -2.959
           
UCC 242.565 -54.979 0.006 -2.883 -2.959
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3592 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=3.2, m-M=15.65, logA=6.2

Search coordinates in Bayestar19

Cluster region map